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The spectral indices of X-ray and radio producing electrons in solar flares
Yao, JX; Yu, XF
1999-04-01
Source PublicationCHINESE ASTRONOMY AND ASTROPHYSICS
ISSN0275-1062
Volume23Issue:2Pages:229-236
AbstractIn the homogeneous model of solar radio burst model, the spectral index of the optically thick part of the spectrum is almost independent of the spectral index of the electron energy, while from the optically thin part, the derived electron index delta(R) is far smaller than that derived from the X-ray emission, delta(X). An inhomogeneous model is proposed, in which, by adjusting two parameters within reasonable limits, we can make delta(R), derived from both the optically thick and thin parts, to equal delta(X). The model is exemplified by the 1981 April 27 0800 UT burst.
KeywordSolar Microwave Burst Hard X-ray Burst Energetic Electrons Spectral Index
Subject AreaAstronomy & Astrophysics
WOS HeadingsScience & Technology ; Physical Sciences
WOS KeywordMICROWAVE BURST SPECTRA
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000083010900013
Citation statistics
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/8323
Collection期刊(老文献)
AffiliationChinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China
Recommended Citation
GB/T 7714
Yao, JX,Yu, XF. The spectral indices of X-ray and radio producing electrons in solar flares[J]. CHINESE ASTRONOMY AND ASTROPHYSICS,1999,23(2):229-236.
APA Yao, JX,&Yu, XF.(1999).The spectral indices of X-ray and radio producing electrons in solar flares.CHINESE ASTRONOMY AND ASTROPHYSICS,23(2),229-236.
MLA Yao, JX,et al."The spectral indices of X-ray and radio producing electrons in solar flares".CHINESE ASTRONOMY AND ASTROPHYSICS 23.2(1999):229-236.
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